Estimates of Proton and Electron Heating Rates Extended to the Near-Sun Environment

Estimates of Proton and Electron Heating Rates Extended to the Near-Sun Environment

A central problem of space plasma physics is how protons and electrons are heated in a turbulent, magnetized plasma. The differential heating of charged species due to dissipation of turbulent fluctuations plays a key role in solar wind evolution. Measurements from previous heliophysics missions hav...

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Váldodahkkit: R. Bandyopadhyay, C. M. Meyer, W. H. Matthaeus, D. J. McComas, S. R. Cranmer, J. S. Halekas, J. Huang, D. E. Larson, R. Livi, A. Rahmati, P. L. Whittlesey, M. L. Stevens, J. C. Kasper, S. D. Bale
Materiálatiipa: Artihkal
Giella:English
Almmustuhtton: IOP Publishing 2023-01-01
Ráidu:The Astrophysical Journal Letters
Fáttát:
Solar wind
Interplanetary physics
Interplanetary turbulence
Solar coronal heating
Magnetohydrodynamics
Liŋkkat:https://doi.org/10.3847/2041-8213/acf85e

Interneahtta

https://doi.org/10.3847/2041-8213/acf85e

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